Stellar kinematics of FCC 167 extracted from the MUSE data (black points) at P.A. = 3.9° within the2 arcsec wide aperture crossing the nucleus shown in Fig. 4. The mean velocity v (bottom panel) and velocity dispersion σ (top panel) are given. The mean errors of the data are shown in the lower-right corner of each panel. The velocity dispersion is compared to the long-slit spectroscopic data obtained by Bedregal et al. (2006) for the north side of the galaxy (red points). The vertical dashed line corresponds to the effective radius.